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Gw170817

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Earth’s gold traces back to ancient neutron-star mergers
science1 month ago

Earth’s gold traces back to ancient neutron-star mergers

Scientists say that most heavy elements like gold were forged in neutron-star mergers via rapid neutron capture, not in ordinary supernovae. The 2017 GW170817 event provided real-time evidence of this process, with gold and other heavy elements ejected in a kilonova and later incorporated into new stars and planets. The gold in our wedding bands, teeth fillings, and heirlooms began its long journey long before the Sun formed, in cosmic collisions that happened billions of years ago.

Cosmic kilonovae forge Earth's gold, GW170817 confirms
science1 month ago

Cosmic kilonovae forge Earth's gold, GW170817 confirms

The 2017 GW170817 neutron‑star collision proved that heavy elements like gold are produced by rapid neutron‑capture (r‑process) in such mergers, ejecting about 6% of a solar mass of material (roughly 20,000 Earth masses) including ~200 Earth masses of gold and ~500 Earth masses of platinum. This material was dispersed through the galaxy before the Solar System formed, explaining why Earth’s gold traces back to ancient stellar explosions. While neutron‑star mergers clearly produce gold, newer analyses suggest they may not account for all galactic heavy elements, with other sources potentially contributing.